A smoother end to the dark ages
arXiv:1104.1189 · doi:10.1038/472047a
Abstract
Independent lines of evidence suggest that the first stars, which ended the cosmic dark ages, came in pairs, rather than singly. This could change the prevailing view that the early Universe had a Swiss-cheese-like appearance.
Nature News and Views, April 7, 2011
References in corpus (5)
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- The Formation of Population III Binaries from Cosmological Initial Conditions
- The formation of the first stars and galaxies
- The first stars: formation of binaries and small multiple systems
- Stellar black holes at the dawn of the universe
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- A simulation calibrated limit on the HI power spectrum from the GMRT Epoch of Reionization experiment
- X-ray Binary Evolution Across Cosmic Time
- Energy Feedback from X-ray Binaries in the Early Universe
- Signatures of X-rays in the early Universe
- Constraining the Statistics of Population III Binaries
- Evidence of Gunn-Peterson damping wings in high-z quasar spectra: strengthening the case for incomplete reionization
- The First Galaxies: Assembly with Black Hole Feedback
- Constraints on X-ray Emissions from the Reionization Era
- Radiative Feedback from high mass X-ray binaries on the formation of the first galaxies and early reionization
- The Aurora radiation-hydrodynamical simulations of reionization: calibration and first results
- Looking at cosmic near-infrared background radiation anisotropies
- Spatially adaptive radiation-hydrodynamical simulations of galaxy formation during cosmological reionization
- Heating the IGM by X-rays from Population III Binaries in High Redshift Galaxies
- The Opacity of the Intergalactic Medium During Reionization: Resolving Small-Scale Structure
- Revisiting The First Galaxies: The epoch of Population III stars
- Spatially Extended 21 cm Signal from Strongly Clustered UV and X-Ray Sources in the Early Universe
- X-ray Background at High Redshifts from Pop III Remnants: Results from Pop III star formation rates in the Renaissance Simulations
- Quasars as probes of cosmological reionization
- Heating and Ionization of the Primordial Intergalactic Medium by High Mass X-ray Binaries
- Modeling the survival of Population III stars till present day
- Black holes at cosmic dawn in the redshifted 21cm signal of HI
- Black Hole High Mass X-ray Binary Microquasars at Cosmic Dawn
- Studying The Effect of Radiation Pressure on Evolution of a Population III Stellar Cluster